反舰导弹智能化作战在线任务分配研究

在预分配基础上,研究反舰导弹多弹协同作战的在线任务重分配.建立了多弹协同任务分配模型,采用基于拍卖协议的一致性方法研究在有中心弹和无中心弹情况下,分布式多弹协同任务重分配.实例仿真结果表明,分布式协同拍卖方法对解决多弹协同任务重分配问题是切实可行的,满足了作战系统对实时性和快速性的要求.     

Decentralized attitude synchronization tracking control for multiple spacecraft under directed communication topology

This paper studies the attitude synchronization tracking control of spacecraft formation flying with a directed communication topology and presents three different controllers. By introducing a novel error variable associated with rotation matrix, a decentralized attitude synchronization controller, which could obtain almost global asymptotical stability of the closed-loop system, is developed. Then, considering model uncertainties and unknown external disturbances, we propose a robust adaptive attitude synchronization controller by designing adaptive laws to estimate the unknown parameters. After that, the third controller is proposed by extending this method to the case of time-varying communication delays via Lyapunov–Krasovskii analysis. The distinctive feature of this work is to address attitude coordinated control with model uncertainties, unknown disturbances and time-varying delays in a decentralized framework, with a strongly connected directed information flow. It is shown that tracking and synchronization of an arbitrary desired attitude can be achieved when the stability condition is satisfied. Simulation results are provided to demonstrate the effectiveness of the proposed control schemes.     

基于LAS码的星群多目标测控技术研究

针对星群多目标同时测控问题,基于星群轨道根数的时延特性和多普勒频移特性分析可得,星群多目标测控的上行链路遥控与测距信号可实现S CDMA（Synchronous Code Division Multiple Access,同步码分多址）,由于星间距离较小,下行链路遥测与测距信号满足QS CDMA（Quasi synchronous code division multiple access,准同步码分多址）.上行链路遥控和测距信号形式设计为PCM BPSK CDMA（Pulse Code Modulation Binary Phase Shift Keying Code Division Multiple Access,脉冲编码调制二进制相移键控码分多址）,上行链路信号采用Gold序列扩频;下行链路遥测和测距信号形式设计为PCM BPSK CDMA,根据总的时延差,提出下行链路采用基于等长脉冲间隔法构造的LAS（Large Area Synchronous,大区域同步）码扩频.结果表明：比特信噪比Eb/N0为10.5 dB时,遥控误码率为1＆#215;10 6;Eb/N0为9.6 dB时,遥测误码率为1×10^5——与达到相同误码性能的Gold序列相比有1 dB改善,因此,LAS码相比于Gold码能够获得更好的误码性能.     

FeAlCrBSiNb非晶涂层形成机理和摩擦磨损行为

研发了一种FeAlCrBSiNb粉芯丝材,采用高速电弧喷涂技术在45钢基体上制备相应涂层.通过SEM,TEM和XRD表征涂层微观组织和相成分,阐述FeAlCrBSiNb非晶涂层的形成机理,利用显微硬度计,万能拉伸试验机和环-块式摩擦磨损试验机,分析涂层力学性能和摩擦磨损行为.结果表明:涂层主要由非晶相和弥散分布其中的α-(Fe),(Fe,Cr),CrB和Fe3Al微晶纳米晶相组成,非晶相体积含量大于91.3％;涂层呈层状结构,结构致密,总体孔隙率约为2％;平均显微硬度值为850 HV0.1,是基体45钢的4倍;优良的磨损抗力使其相对耐磨性是45钢的5倍,其磨损机制主要为剥落引起的剥落磨损.     

无人机编队飞行技术的研究现状与展望

无人机编队飞行是无人机及其应用技术发展研究的新热点.在分析无人机编队飞行特点的基础上,阐述了无人机编队飞行原理与方法的研究现状,并展望了其今后的主要应用前景.     

Formation and Composition of Planetesimals

The composition of planetesimals depends upon the epoch and the location of their formation in the solar nebula. Meteorites produced in the hot inner nebula contain refractory compounds. Volatiles were present in icy planetesimals and cometesimals produced in the cold outer nebula. However, the mechanism responsible for their trapping is still controversial. We argue for a general scenario valid in all regions of the turbulent nebula where water condensed as a crystalline ice (Hersant et al., 2004). Volatiles were trapped in the form of clathrate hydrates in the continuously cooling nebula. The epoch of clathration of a given species depends upon the temperature and the pressure required for the stability of the clathrate hydrate. The efficiency of the mechanism depends upon the local amount of ice available. This scenario is the only one so far which proposes a quantitative interpretation of the non detection of N₂ in several comets of the Oort cloud (Iro et al., 2003). It may explain the large variation of the CO abundance observed in comets and predicts an Ar/O ratio much less than the upper limit of 0.1 times the solar ratio estimated on C/2001 A2 (Weaver et al., 2002). Under the assumption that the amount of water ice present at 5 AU was higher than the value corresponding to the solar O/H ratio by a factor 2.2 at least, the clathration scenario reproduces the quasi uniform enrichment with respect to solar of the Ar, Kr, Xe, C, N and S elements measured in Jupiter by the Galileo probe. The interpretation of the non-uniform enrichment in C, N and S in Saturn requires that ice was less abundant at 10 AU than at 5 AU so that CO and N₂ were not clathrated in the feeding zone of the planet while CH₄, NH₃ and H₂S were. As a result, the 14N/15N ratio in Saturn should be intermediate between that in Jupiter and the terrestrial ratio. Ar and Kr should be solar while Xe should be enriched by a factor 17. The enrichments in C, N and S in Uranus and Neptune suggest that available ice was able to form clathrates of CH₄, CO and the NH₃ hydrate, but not the clathrate of N₂. The enrichment of oxygen by a factor 440 in Neptune inferred by Lodders and Fegley (1994) from the detection of CO in the troposphere of the planet is higher by at least a factor 2.5 than the lower limit of O/H required for the clathration of CO and CH4 and for the hydration of NH₃. If CO detected by Encrenaz et al. (2004) in Uranus originates from the interior of the planet, the O/H ratio in the envelope must be around of order of 260 times the solar ratio, then also consistent with the trapping of detected volatiles by clathration. It is predicted that Ar and Kr are solar in the two planets while Xe would be enriched by a factor 30 to 70. Observational tests of the validity of the clathration scenario are proposed.     

原位钛基复合材料中TiB的生成热力学及动力学

采用自蔓延高温合成（SHS）、感应熔炼和熔模精铸相结合的方法，利用Ti—B—Al体系制备出了原位自生TiB增强的钛基复合材料。借助XRD、SEM和TEM分析了复合材料的物相和增强体的形态。结果表明：在复合材料中只存在TiB增强体和Ti，无TiAl3杂质相形成，TiB增强体呈柱状短纤维，这与其B27晶体结构有关，且增强体／基体界面清洁无杂质污染，并从热力学和动力学两方面论述了在Ti—B—Al体系中制备TiB增强体的生成机制：在Ti-B—Al体系中，Al首先受热熔化使得Ti和B相继溶解于Al液中；Ti与Al之间先行发生化学反应形成Ti—Al金属间化合物，放出的热量进一步引发了溶解于液相中的B和Ti产生高温自蔓延形成Ti—B化合物。以热力学理论分析，应最终形成TiB2，但实际上由于动力学影响，最终形成了TiB。     

对舰面温度数据的建模及其趋势和周期性分析

在系统建模理论的基础上,运用改进的动态数据建模方法,文章对某舰面温度数据进行建模并验证了模型的适用性,然后根据建立的模型进行了趋势和周期性分析。根据模型的适用性检验发现,对所研究的温度数据而言,ARMA(6,5)模型是最合适的,且其具有一定的线性趋势,但周期性不很明显。所有的建模和分析过程均在MATLAB上实现。     

L10-TiAl金属间化合物Mn,Nb合金化电子结构的计算

采用第一原理赝势平面波方法计算了L10型TiAl金属间化合物中掺入Mn,Nb后的电子结构和价键结构.通过合金原子形成热得出Mn优先占据Al点阵位置,Nb优先占据Ti点阵位置.Mulliken聚居数分析发现Mn或Nb合金化后,分别降低了(001)和(002)面内的原子间键合强度,掺入Nb还降低了层间的原子间键合强度,而掺入Mn,则使层间原子间键合强度增加.整体上来讲,掺入Mn有利于改善TiAl的室温脆性,而掺入Nb,不利于改善TiAl的室温脆性.     

铰接式旋翼舰面瞬态气弹响应及参数研究

为了研究舰面铰接式旋翼桨叶桨尖与机体相碰的原因及参数影响,本文采用中等变形梁模型处理桨叶弹性变形,用有限转角模拟桨叶绕铰刚性运动和非线性准定常气动模型处理气动力。通过与国外计算及试验数据的相关性分析,验证了本文建模及计算方法的正确性。参数分析表明:1)挥舞限动块脱开前,桨叶弹性变形提供的桨尖挥舞位移占主要部分,脱开后,桨叶刚性运动提供的桨尖挥舞位移占主要部分;2)舰面流场采用梯形流时,计算的桨尖挥舞位移最大;3)挥舞限动角大小及离心式限动块释放时间对桨尖最大挥舞位移影响不明显;4)直接增加桨叶挥舞刚度可显著地减小桨尖向下最大挥舞位移;5)随总距增加,桨尖挥舞挠度减小不明显,这是通过增加总距来减小桨叶挥舞位移不可行的另一原因。